ScopeX Asteroids Followup Throop Oct14 - ASSA
Transcription
ScopeX Asteroids Followup Throop Oct14 - ASSA
Amateur Observations of Near-Earth Asteroids from South Africa Henry Throop! Physics Department, University of Pretoria Planetary Science Institute, Tucson, USA 1 Oct 2014 Inventory of Earth Impactors Megatons TNT Total Detected South African Airburst (1963) Chelyabinsk (2013) Small; Protected! by Earth’s ! Atmosphere Tunguska (1908) Large; Nearly All Detected Dangerous and Not Yet Detected! Impact Interval [years] Number, N < D Hiroshima K-T Impactor (65 Mya) Vredefort (2.2 Gya) Absolute Magnitude H Assumes albedo 0.14 Diameter [km] NEAs only All asteroids Asteroid Type # Known Main-Belt Asteroids 500,000 Near-Earth Asteroids (NEAs) Pass within 0.1 AU of Earth 11,000 Potentially Hazardous Asteroids (PHAs) Cross Earth orbit and r > 100 m 1400 How to Handle the Asteroid Risk? ! ! Asteroid Grand Challenge NASA must “find all asteroid threats to human populations and know what to do about them.”! • Detect all NEAs > 100 m! • Characterize them! • Determine a way to mitigate them! US Congress, July 2013 11 time zones Observatory with reported NEA observations There is a huge gap in global observational coverage of asteroids… and it is centered on South Africa, which has a lot of telescopes! How to Detect and Characterize Asteroids MIT LINEAR New Mexico Catalina Sky Survey Arizona & Australia Pan-STARRS Hawaii • 1m - 2m wide-angle robotic telescopes have been very successful for detection: nearly 95% of all suspected NEAs > 1 km have now been detected. • But the vast majority of the NEOs discovered in these searches are never observed again! We know nothing about their shape, rotation rate, possible binaries, composition, size, etc.! • This is where amateurs with access to moderate facilities can play a key role. ! • Measuring rotational light curves (~4-12 hours) of NEOs when near periapse! • Measuring positions of NEOs in the few weeks post-discovery for improved orbits. Asteroid 3288 Selucus! NEA, perihelion 1.1 AU, e = 0.45, H=15.3, v = 17, discovered 1982 We measure light curve to determine rotation rate, shape, binarity of asteroid. ! Vast majority of NEAs have never been studied post-discovery. June 2014, SAAO 1m Throop / Reddy / Morris How South Africa can play a role ! in the Asteroid Grand Challenge and NEA studies Discovering new NEAs Requires wide-angle robotic telescopes Immediate followup post-discovery; Geographic advantage of SA orbital measurements fills major hole. Characterization: Shape, spin rate, Ready access to moderate telescopes (<1m). composition Closing Thoughts Impact risk is a non-negligible threat to humanity, of great interest to NASA and other countries. ! The majority of potentially hazardous asteroids (PHAs) have not yet been discovered… and of those known, the majority have never been studied. ! South African amateurs can make significant contributions to important science. ! Thank you! [email protected]